Effects of variable sedimentation rates and age errors on the resolution of sedimentary paleointensity records

被引:24
作者
Guyodo, Y [1 ]
Channell, JET [1 ]
机构
[1] Univ Florida, Dept Geol Sci, Gainesville, FL 32611 USA
关键词
paleomagnetism; magnetic intensity; timescales; numerical models; time series analysis; 1560 geomagnetism and paleomagnetism : time variations-secular and long term; 3210 mathematical geophysics : modeling;
D O I
10.1029/2001GC000211
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
[1] Synthetic, u-channel records of relative paleointensity have been generated with a numerical model simulating the recording process in sediments, variable quality age control and variable sedimentation rates, over a time interval of 500 ky. Simulation results indicate that paleointensity records with mean sedimentation rates up to 15 cm/ky can reflect geomagnetic dipole intensity fluctuations, with some amplitude differences between individual records of nongeomagnetic origin. This study confirms that relative paleointensity records have great potential as a stratigraphic tool and that a stratigraphic precision of a few thousand years can be achieved with records characterized by high sedimentation rates. Spectral analyses suggest that caution should be used when interpreting the power spectra of individual records and that stacked records should be favored. Stacked u-channel records with mean sedimentation rates of 1 cm/ky do not provide reliable spectral information on the dipole intensity for wavelengths shorter than 25-50 ky, and their utility is limited to long-term trends in paleointensity. For higher sedimentation rates, the range of spectral information depends on the stack resolution (sedimentation rates) and the age model. The best results are, predictably, obtained with high sedimentation rates and excellent age control. In these cases, the power spectra are reliable for wavelengths as short as 4 ky.
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页数:18
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共 50 条
[1]   Orbital modulation of the Earth's magnetic field intensity [J].
Channell, JET ;
Hodell, DA ;
McManus, J ;
Lehman, B .
NATURE, 1998, 394 (6692) :464-468
[2]   Relative geomagnetic paleointensity and δ18O at ODP Site 983 (Gardar Drift, North Atlantic) since 350 ka [J].
Channell, JET ;
Hodell, DA ;
Lehman, B .
EARTH AND PLANETARY SCIENCE LETTERS, 1997, 153 (1-2) :103-118
[3]   Geomagnetic paleointensity for the last 100 kyr from the sub-antarctic South Atlantic: a tool for inter-hemispheric correlation [J].
Channell, JET ;
Stoner, JS ;
Hodell, DA ;
Charles, CD .
EARTH AND PLANETARY SCIENCE LETTERS, 2000, 175 (1-2) :145-160
[4]   Geomagnetic palaeointensities and astrochronological ages for the Matuyama-Brunhes boundary and the boundaries of the Jaramillo Subchron: palaeomagnetic and oxygen isotope records from ODP Site 983 [J].
Channell, JET ;
Kleiven, HF .
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY OF LONDON SERIES A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 2000, 358 (1768) :1027-1047
[5]   STATISTICS OF THE GEOMAGNETIC SECULAR VARIATION FOR THE PAST 5-MY [J].
CONSTABLE, CG ;
PARKER, RL .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1988, 93 (B10) :11569-11581
[6]   DEPTH OF POSTDEPOSITIONAL REMANENCE ACQUISITION IN DEEP-SEA SEDIMENTS - A CASE-STUDY OF THE BRUNHES-MATUYAMA REVERSAL AND OXYGEN ISOTOPIC STAGE-19.1 [J].
DEMENOCAL, PB ;
RUDDIMAN, WF ;
KENT, DV .
EARTH AND PLANETARY SCIENCE LETTERS, 1990, 99 (1-2) :1-13
[7]  
Dormy E, 2000, GEOCHEM GEOPHY GEOSY, V1
[8]   Relative variations in geomagnetic intensity from sedimentary records: The past 200,000 years [J].
Guyodo, Y ;
Valet, JP .
EARTH AND PLANETARY SCIENCE LETTERS, 1996, 143 (1-4) :23-36
[9]   A sedimentary paleomagnetic record of the Matuyama chron from the Western Antarctic margin (ODP Site 1101) [J].
Guyodo, Y ;
Acton, GD ;
Brachfeld, S ;
Channell, JET .
EARTH AND PLANETARY SCIENCE LETTERS, 2001, 191 (1-2) :61-74
[10]   Paleointensity record from Pleistocene sediments (1.4-0 Ma) off the California Margin [J].
Guyodo, Y ;
Richter, C ;
Valet, JP .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH, 1999, 104 (B10) :22953-22964